In this work, we go a step further and study how different AGN contributions may affect the six
morphological parameters that are commonly used in non-parametric
methods for galaxy classification. We carried out all the analysis by
using a sample of a number of local, non-active galaxies with known visual
morphological classification [1]}. In this paper, we
present the results obtained for the original sample at
z \(\sim \)  0. The simulations at fainter magnitudes
and higher redshifts will be presented in a forthcoming paper
(Getachew et al., in prep.).
